Star Formation from Low-metallicity Gas

摘要：

We present the thermal evolution of low-metallicity clouds and consider their fragmentation mass scales. Then, we study the protostellar evolution in the main accretion phase, and discuss the upper limit on the stellar mass by the stellar feedback.

关键词： stars formation stars Population Ⅱ

作者: Kazuyuki Omukai

作者单位: National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

会议类型: 国际会议

会议名称: The 10th Asian-Pacific Regional International Astronomical Union Meeting(第十届亚洲及太平洋地区天文学大会 APRIM)

会议地点: 昆明

会议语种:英文

页码: 150-152

在线出版日期: 2008-08-03（万方平台首次上网日期，不代表论文的发表时间）